1k citations · 1.7k across the 21 of their papers we have counts for
21 papers
Shell helium-burning hot subdwarf B stars as candidates for blue large-amplitude pulsators
H. Xiong, L. Casagrande, X. Chen +7
Blue large-amplitude pulsators (BLAPs) are a newly discovered type of variable star. Their typical pulsation periods are on the order of a few tens of minutes, with relatively larg…
Type Ia supernova ejecta-donor interaction: explosion model comparison
C. McCutcheon, Y. Zeng, Z. -W. Liu +4
In the single-degenerate scenario of Type Ia supernovae (SNe Ia), the interaction between high-speed ejected material and the donor star in a binary system is expected to lead to m…
Predicting the amount of hydrogen stripped by the supernova explosion for SN 2002cx-like SNe Ia
Zheng-Wei Liu, M. Kromer, M. Fink +5
The most favored progenitor scenarios for Type Ia supernovae (SNe Ia) involve the single-degenerate (SD) scenario and the double-degenerate scenario. The absence of stripped hydrog…
A progenitor binary and an ejected mass donor remnant of faint type Ia supernovae
S. Geier, T. R. Marsh, B. Wang +17
Type Ia supernovae (SN Ia) are the most important standard candles for measuring the expansion history of the universe. The thermonuclear explosion of a white dwarf can explain the…
Double-detonation explosions as progenitors of type Iax supernovae
Bo Wang, Stephen Justham, Zhanwen Han
It has recently been proposed that one sub-class of type Ia supernovae (SNe Ia) is sufficiently both distinct and common to be classified separately from the bulk of SNe Ia, with a…
Effects of tidally enhanced stellar wind on the horizontal branch morphology of globular clusters
Zhen-Xin Lei, Xue-Fei Chen, Feng-Hui Zhang +1
Metallicity is the first parameter to influence the horizontal branch (HB) morphology of globular clusters (GCs). It has been found, however, that some other parameters may also pl…